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Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches
Shternin, P.1; Kirichenko, A.1,2; Zyuzin, D.1; Yu, M.3; Danilenko, A.1; Voronkov, M.4; Shibanov, Yu.1
刊名ASTROPHYSICAL JOURNAL
2019-06-01
卷号877期号:2页码:15
关键词ISM: individual objects (RCW 114) ISM: supernova remnants pulsars: general pulsars: individual (PSR J1731-4744)
ISSN号0004-637X
DOI10.3847/1538-4357/ab1905
英文摘要The bright radio pulsar B1727-47, with a characteristic age of 80 kyr, was among the first pulsars discovered 50 yr ago. Using regular timing observations and its interferometric positions at three epochs, we measured, for the first time, the pulsar proper motion of 151 +/- 19 mas yr(-1). At the dispersion measure distance of greater than or similar to 2.7 kpc, this would suggest a record transverse velocity of the pulsar of greater than or similar to 1900 km s(-1). However, a backward extrapolation of the pulsar track to its birth epoch points remarkably close to the center of the evolved nearby supernova remnant RCW 114, which suggests genuine association of the two objects. In this case, the pulsar is substantially closer (similar to 0.6 kpc) and younger (similar to 50 kyr), and its velocity (similar to 400 km s(-1)) is compatible with the observed pulsar velocity distribution. We also identified two new glitches of the pulsar. We discuss implications of our results for the properties of the pulsar and the remnant.
资助项目Australian Government
WOS关键词CORE-COLLAPSE SUPERNOVAE ; TIMING OBSERVATIONS ; FILAMENTARY NEBULA ; NEUTRON-STARS ; PACKAGE ; SIMULATIONS ; DYNAMICS ; PERIODS ; TEMPO2 ; SINGLE
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000469433800014
资助机构Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government ; Australian Government
内容类型期刊论文
源URL[http://ir.bao.ac.cn/handle/114a11/26457]  
专题中国科学院国家天文台
通讯作者Shternin, P.
作者单位1.Ioffe Inst, Politekhnicheskaya 26, St Petersburg 194021, Russia
2.Univ Nacl Autonoma Mexico, Inst Astron, Apdo Postal 877, Ensenada 22800, Baja California, Mexico
3.Chinese Acad Sci, Natl Astron Observ, Beijing, Peoples R China
4.CSIRO Astron & Space Sci, POB 76, Epping, NSW 1710, Australia
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GB/T 7714
Shternin, P.,Kirichenko, A.,Zyuzin, D.,et al. Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches[J]. ASTROPHYSICAL JOURNAL,2019,877(2):15.
APA Shternin, P..,Kirichenko, A..,Zyuzin, D..,Yu, M..,Danilenko, A..,...&Shibanov, Yu..(2019).Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches.ASTROPHYSICAL JOURNAL,877(2),15.
MLA Shternin, P.,et al."Tracking the Footprints of the Radio Pulsar B1727-47: Proper Motion, Host Supernova Remnant, and the Glitches".ASTROPHYSICAL JOURNAL 877.2(2019):15.
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